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2122 Pyatiletka

From Wikipedia, the free encyclopedia
Stony asteroid

2122 Pyatiletka
Discovery[1]
Discovered byT. Smirnova
Discovery siteCrimean Astrophysical Obs.
Discovery date14 December 1971
Designations
(2122) Pyatiletka
Named after
Pyatiletka
(Five-year plans of the USSR)[2]
1971 XB · 1950 BE1
1950 DX · 1951 KB1
1954 DA · 1961 AL
1969 EV1
main-belt · (inner)[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc63.18 yr (23,075 days)
Aphelion2.4729AU
Perihelion2.3310 AU
2.4019 AU
Eccentricity0.0295
3.72yr (1,360 days)
197.74°
0° 15m 53.28s / day
Inclination7.8981°
105.50°
236.47°
Physical characteristics
Dimensions10.75 km(calculated)[3]
11.00±0.83 km[4]
11.084±0.101 km[5]
11.554±0.074 km[6]
8.899±0.0053h[7]
0.1931±0.0198[6]
0.20(assumed)[3]
0.211±0.033[4]
0.224±0.023[5]
S[3]
11.759±0.002(R)[7] · 12.1[1][4][6] · 12.21[3] · 12.40±0.29[8]

2122 Pyatiletka, provisional designation1971 XB, is a stonyasteroid from the inner regions of theasteroid belt, approximately 11 kilometers in diameter.

The asteroid was discovered on 14 December 1971 by Soviet astronomerTamara Smirnova at theCrimean Astrophysical Observatory in Nauchnyj, on the Crimean peninsula.[9] It was named for "pyatiletka", the firstFive-Year Plan of the USSR.[2]

Orbit and classification

[edit]

Pyatiletka orbits the Sun in theinner main-belt at a distance of 2.3–2.5 AU once every 3 years and 9 months (1,360 days). Its orbit has aneccentricity of 0.03 and aninclination of 8° with respect to theecliptic.[1]

It was first identified as1950 BE1 atSimeiz Observatory in 1950. The body'sobservation arc begins atLowell Observatory in 1961, when it was identified as1961 AL, 10 years prior to its official discovery observation at Nauchnyj.[9]

Physical characteristics

[edit]

Pyatiletka has been characterized as a stonyS-type asteroid.[3]

Lightcurves

[edit]

A fragmentary rotationallightcurve ofPyatiletka was obtained from photometric observations at thePalomar Transient Factory in California in February 2010. Lightcurve analysis gave a tentativerotation period of 8.899 hours with a brightness variation of 0.10magnitude (U=1).[7] As of 2017, no other lightcurve has been published.[3]

Diameter and albedo

[edit]

According to the surveys carried out by the JapaneseAkari satellite and NASA'sWide-field Infrared Survey Explorer with its subsequentNEOWISE mission,Pyatiletka measures between 11.00 and 11.55 kilometers in diameter, and its surface has analbedo between 0.1931 and 0.224.[4][5][6] TheCollaborative Asteroid Lightcurve Link assumes a standard albedo for stony asteroids of 0.20 and calculates a diameter of 10.75 kilometers with anabsolute magnitude of 12.21.[3]

Naming

[edit]

Thisminor planet was named in honor of thefive-year plans of the Soviet Union on the occasion of the 50th anniversary of itsfirst adoption.[2] The official naming citation was published by theMinor Planet Center on 1 April 1980 (M.P.C. 5283).[10]

References

[edit]
  1. ^abcd"JPL Small-Body Database Browser: 2122 Pyatiletka (1971 XB)" (2017-04-30 last obs.).Jet Propulsion Laboratory. Retrieved11 June 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(2122) Pyatiletka".Dictionary of Minor Planet Names – (2122) Pyatiletka.Springer Berlin Heidelberg. p. 172.doi:10.1007/978-3-540-29925-7_2123.ISBN 978-3-540-00238-3.
  3. ^abcdefgh"LCDB Data for (2122) Pyatiletka". Asteroid Lightcurve Database (LCDB). Retrieved27 March 2017.
  4. ^abcdUsui, Fumihiko; Kuroda, Daisuke; Müller, Thomas G.; Hasegawa, Sunao; Ishiguro, Masateru; Ootsubo, Takafumi; et al. (October 2011)."Asteroid Catalog Using Akari: AKARI/IRC Mid-Infrared Asteroid Survey".Publications of the Astronomical Society of Japan.63 (5):1117–1138.Bibcode:2011PASJ...63.1117U.doi:10.1093/pasj/63.5.1117. (online,AcuA catalog p. 153)
  5. ^abcMasiero, Joseph R.; Grav, T.; Mainzer, A. K.; Nugent, C. R.; Bauer, J. M.; Stevenson, R.; et al. (August 2014)."Main-belt Asteroids with WISE/NEOWISE: Near-infrared Albedos".The Astrophysical Journal.791 (2): 11.arXiv:1406.6645.Bibcode:2014ApJ...791..121M.doi:10.1088/0004-637X/791/2/121. Retrieved27 March 2017.
  6. ^abcdMainzer, A.; Grav, T.; Masiero, J.; Hand, E.; Bauer, J.; Tholen, D.; et al. (November 2011). "NEOWISE Studies of Spectrophotometrically Classified Asteroids: Preliminary Results".The Astrophysical Journal.741 (2): 25.arXiv:1109.6407.Bibcode:2011ApJ...741...90M.doi:10.1088/0004-637X/741/2/90.
  7. ^abcWaszczak, Adam; Chang, Chan-Kao; Ofek, Eran O.; Laher, Russ; Masci, Frank; Levitan, David; et al. (September 2015)."Asteroid Light Curves from the Palomar Transient Factory Survey: Rotation Periods and Phase Functions from Sparse Photometry".The Astronomical Journal.150 (3): 35.arXiv:1504.04041.Bibcode:2015AJ....150...75W.doi:10.1088/0004-6256/150/3/75. Retrieved27 March 2017.
  8. ^Veres, Peter; Jedicke, Robert; Fitzsimmons, Alan; Denneau, Larry; Granvik, Mikael; Bolin, Bryce; et al. (November 2015)."Absolute magnitudes and slope parameters for 250,000 asteroids observed by Pan-STARRS PS1 - Preliminary results".Icarus.261:34–47.arXiv:1506.00762.Bibcode:2015Icar..261...34V.doi:10.1016/j.icarus.2015.08.007. Retrieved27 March 2017.
  9. ^ab"2122 Pyatiletka (1971 XB)".Minor Planet Center. Retrieved27 March 2017.
  10. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved27 March 2017.


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